CWNU 1130
Summary
CWNU 1130 is a poorly populated, moderately dense object of low C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It was recently reported in the literature.
This object shares a significant percentage of members with a later reported entry.
Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2022) | 49.062 | 60.591 | 0.934 | 0.335 | 0.676 | – |
| UCC | 49.037 | 60.602 | 0.932 | 0.34 | 0.675 | -24.929 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | A0=1.85, logAge=7.15 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Theia 1740 | 65.7 | 49.25 | 60.54 | 0.94 | 0.34 | 0.64 | -13.46 | 0.04 |